Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/36350
Title: | X-Ray Polarimetry of the Crab Nebula with PolarLight: Polarization Recovery after the Glitch and a Secular Position Angle Variation | Authors: | Long, Xiangyun Feng, Hua Li, Hong Zhu, Jiahuan Wu, Qiong Huang, Jiahui Minuti, Massimo Jiang, Weichun Wang, Weihua Xu, Renxin COSTA, ENRICO Yang, Dongxin Citraro, Saverio Nasimi, Hikmat Yu, Jiandong Jin, Ge Zeng, Ming An, Peng Baldini, Luca Bellazzini, Ronaldo Brez, Alessandro Latronico, Luca Sgrò, Carmelo Spandre, Gloria Pinchera, Michele MULERI, FABIO SOFFITTA, PAOLO |
Issue Date: | 2021 | Journal: | THE ASTROPHYSICAL JOURNAL LETTERS | Number: | 912 | Issue: | 2 | First Page: | L28 | Abstract: | We report follow-up observations of the Crab Nebula with the PolarLight X-ray polarimeter, which revealed a possible variation in polarization associated with a pulsar glitch in 2019. The new observations confirm that the polarization has recovered roughly 100 days after the glitch. With the new observations, we find that the polarization angle (PA) measured with PolarLight from the total nebular emission has a difference of 18°0 ± 4°6 from that measured 42 yr ago with OSO-8, indicating a secular evolution of polarization with either the Crab Nebula or pulsar. The long-term variation in PA could be a result of multiple glitches in the history, magnetic reconnection, or movement of synchrotron emitting structures in the nebula, or secular evolution of the pulsar magnetic geometry. | URI: | http://hdl.handle.net/20.500.12386/36350 | URL: | https://api.elsevier.com/content/abstract/scopus_id/85106340894 https://iopscience.iop.org/article/10.3847/2041-8213/abfb00 |
ISSN: | 2041-8205 | DOI: | 10.3847/2041-8213/abfb00 | Bibcode ADS: | 2021ApJ...912L..28L | Fulltext: | open |
Appears in Collections: | 1.01 Articoli in rivista |
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2021_ApJL_Long.pdf | pdf editoriale | 322.71 kB | Adobe PDF | View/Open |
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